Open Access
Table 7
Comparison of the orbital parameters HD 121056 b and c from different studies.
Parameter | Unit | Jones et al. 2015b | Wittenmyer et al. 2015 | Feng et al. 2022 | This work |
---|---|---|---|---|---|
Pb | (days) | 88.9 ± 0.1 | 89.09 ± 0.11 | ![]() |
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Kb | (m s−1) | 45.5 ± 1.6 | 47.9 ± 11.0 | ![]() |
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eb | 0.05 ± 0.04 | 0.06 ± 0.04 | ![]() |
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|
ωb | (deg) | 138 ± 60 | 300 ± 132 | ![]() |
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TPb | (JD − 2 450 000) | 2997.8 ± 16.7 | 4810 ± 33 | ![]() |
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mb sin ib | (MJup) | 1.38 ± 0.15 | 1.25 ± 0.04 | ![]() |
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Pc | (days) | 2131.8 ± 88.3 | 2203 ± 486 | ![]() |
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Kc | (m s−1) | 69.0 ± 3.3 | 81.9 ± 14.0 | ![]() |
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ec | 0.17 ± 0.06 | 0.18 ± 0.07 | ![]() |
![]() |
|
ωc | (deg) | 166.5 ± 20.5 | 205 ± 17 | ![]() |
![]() |
TPc | (JD − 2 450 000) | 2684.1 ± 235.7 | 3068 ± 405 | ![]() |
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mc sin ic | (MJup) | 5.98 ± 0.76 | 6.14 ± 1.99 | ![]() |
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Notes. For the solution of Wittenmyer et al. (2015), we only show here the results obtained with the “bootstrap solution” of the combined analysis (using FEROS, CHIRON, and UCLES) in the paper.
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